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locally and globally to examine water quality, chemical composition of dissolved
organic matter, trace water masses and study dynamical processes involving CDOM.
CDOM
cant inelastic process in natural waters, along with
vibrational Raman scattering (VRS) and chlorophyll
fl
fluorescence is a signi
uorescence.
Between processes of absorption and emission some energy is dissipated, so the
energy emitted is lower than the energy absorbed. The wavelengths at which a
photon is absorbed and emitted depend mainly on the molecule itself, but can also
depend on several environmental factors, e.g. pH, temperature, a presence of certain
metals (Hudson et al. 2007 ). Fluorescent CDOM is a complex mixture of many
fl
fl
fluorescent compounds, and individual
fluorophores are hard to identify.
Because of the shift of wavelength in the
fl
fluorescence process, its effect on the
backscattered radiation at the top of atmosphere is possibly identi
fl
lling-
in of Fraunhofer lines, which are spectrally narrow, often saturated absorption
features in the solar spectrum. Other inelastic processes have been already retrieved
from hyperspectral satellite data with the Differential Optical Absorption Spec-
troscopy (DOAS) method (e.g. Vountas et al. 1998 , 2003 , 2007 ). In this work we
test the use of the
ed in the
uorescence to char-
acterize CDOM composition and concentration independent from chlorophyll. This
method would also help to improve chlorophyll retrievals in regions of high CDOM
concentrations.
filling-in signal originating from CDOM
fl
2 Methods
2.1 DOAS Retrieval Technique
Different variants of the DOAS technique have been applied for several years for
the retrieval of atmospheric trace gases from satellite measurements (e.g. Burrows
et al. 1999 ; Richter et al. 2005 ), and have lately been extended to the aquatic
domain as PhytoDOAS (Vountas et al. 2007 : Bracher et al. 2009 ; Sadeghi et al.
2012 ). The DOAS method is based on Beer-Lambert
is law (e.g. Rozanov and
Rozanov 2010 ) and determines the amount of molecular absorbers along the
effective optical light path by
'
fitting and scaling spectra within a given wavelength
window. The broad-band effects (e.g. Rayleigh and Mie scattering) are removed by
a low-degree polynomial that is also
fitting in the DOAS method is
formalized as a least-squares minimization and is described by the following
equation:
tted. The
2
X
N
n¼1 r n ðkÞ S n r R ðkÞ S R r V ðkÞ S V r f ðkÞ S f
X
M
m
sðkÞ
a m k
! min : ð
1
Þ
m¼0
ln I ðkÞ
I 0 ðkÞ
are
the measured backscattered radiance and extraterrestrial irradiance, respectively;
Here,
sðkÞ ¼
is the so-called slant optical density,
I ðkÞ
and I 0 ðkÞ
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